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Volumn 18, Issue 8, 1996, Pages 213-216

Factors controlling the shape and size of the post-terminator magnetopause

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EID: 0042538701     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00963-9     Document Type: Article
Times cited : (2)

References (13)
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  • 5
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    • (1969) Planet. Space Sci. , vol.17 , pp. 233-246
    • Spreiter, J.R.1    Alksne, A.Y.2
  • 6
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    • F. V. Coroniti and C. F. Kennel, Changes in magnetospheric configuration during the substorm growth phase, J. Geophys. Res., 77, 3361-3370, 1972.
    • (1972) J. Geophys. Res. , vol.77 , pp. 3361-3370
    • Coroniti, F.V.1    Kennel, C.F.2
  • 7
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    • Solar wind influence on magnetotail configuration and dynamics
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    • (1986) Solar Wind-Magnetosphere Coupling , pp. 671-690
    • Lui, A.T.Y.1
  • 8
    • 0041401829 scopus 로고
    • IMP 8 magnetic observations of the high-latitude boundary: Locations and force balance
    • S. Ohtani and S. Kokubun, IMP 8 magnetic observations of the high-latitude boundary: locations and force balance, J. Geophys. Res., 95, 20759-20769, 1990.
    • (1990) J. Geophys. Res. , vol.95 , pp. 20759-20769
    • Ohtani, S.1    Kokubun, S.2
  • 9
    • 0001721782 scopus 로고
    • Solar wind control of the magnetopause shape, location, and motion
    • D. G. Sibeck, R. E. Lopez, and E. C. Roelof, Solar wind control of the magnetopause shape, location, and motion, J. Geophys. Res., 96, 5489-5495, 1991.
    • (1991) J. Geophys. Res. , vol.96 , pp. 5489-5495
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  • 11
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    • An empirical model of the size and shape of the near-Earth magnetotail
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    • (1993) Geophys. Res. Letts. , vol.20 , pp. 2695-2698
    • Petrinec, S.M.1    Russell, C.T.2
  • 12
    • 0041401830 scopus 로고
    • The near-Earth magnetotail shape and size as determined from the magnetopause flaring angle
    • June
    • S. M. Petrinec and C. T. Russell, The near-Earth magnetotail shape and size as determined from the magnetopause flaring angle, submitted to J. Geophys. Res., June, 1994.
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  • 13
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    • Factors which control the size of the magnetosphere
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